The Reionization Epoch Bright Emission Line Survey (REBELS) is an ALMA Large Programme targeting [OIII] and [CII] lines and their underlying dust continuum (at \(\sim 90\)  and \(160\mu \) m) in 40 UV-bright LBGs at \(z>6.5\)  [1]}. From this sample, 18 sources have been detected in the continuum so far [2]}, which more than tripled the previous number of dust continuum detections at \(z>6.5\) . The inferred infrared luminosities of these continuum-detected sources imply that about half of their star formation is dust-obscured. One of the detections, REBELS-25, is noteworthy as it is an ultra-luminous infrared galaxy (ULIRG, with \(L_\mathrm {IR}>10^{12}\,L_\odot \) ) at \(z=7.4\)  (Hygate et al., submitted).
